（1）Zhang X., Jeffery C. S., Li Y., Bi S., Population Synthesis of Helium White Dwarf-Red Giant Star Mergers and the Formation of Lithium-rich Giants and Carbon Stars, ApJ, 2020, 889, 33
（2）Zhang X., Gao H., What binary systems are the most likely sources for periodically repeating FRBs?, MNRAS, 2020, 498, L1
（3）Zhang X., Hall P. D., Jeffery C. S., Bi S., Evolution models of helium white dwarf–main-sequence star merger remnants: the mass distribution of single low-mass white dwarfs，2018, MNRAS, 474,427
（4）Zhang X., Liu J., Jeffery C. S., Hall P. D., Bi S., The double helium-white dwarf channel for the formation of AM CVn binaries，2018, RAA, 18, 9Z
（5）Zhang X., Hall P. D., Jeffery C. S., Bi S., Evolution Models of Helium White Dwarf–Main-sequence Star Merger Remnants，2017, ApJ, 835, 242
（6）Zhang X., Jeffery C. S., Chen X., Han Z., Post-merger evolution of carbon-oxygen + helium white dwarf binaries and the origin of R Coronae Borealis and extreme helium stars, 2014, MNRAS, 445, 660
(7) Zhang X., Jeffery C. S., White dwarf-red giant mergers, early-type R stars, J stars and lithium, 2013, MNRAS, 430,2113
（8）Zhang X., Jeffery C. S., Can R Coronae Borealis stars form from the merger of two helium white dwarfs? 2012, MNRAS, 426, L81
（9）Zhang X., Jeffery C. S., Evolutionary models for double helium white dwarf mergers and the formation of helium-rich hot subdwarfs, 2012, MNRAS, 419, 452
（10）Zhang X., Chen X., Han Z., The masses of hot subdwarfs, 2009, A&A, 504, L13
